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Using our previously reported observations, we derive some physicalparameters of the moderately fast nova V2676 Ophiuchi 2012 # 1. The best-fitCLOUDY model of the nebular spectrum obtained on 2015 May 8 shows a hot whitedwarf source with Tbb = 1.0 x 10^{5} K having a luminosity of 1.0 x 10^{38}ergs/s. Our abundance analysis shows that the ejecta are significantly enhancedrelative to solar, He/H = 2.14, O/H = 2.37, S/H = 6.62 and Ar/H = 3.25. Theejecta mass is estimated to be 1.42 x 10^{-5} Msun. The nova showed apronounced dust formation phase after 90 days from discovery. The J-H and H-Kcolors were very large as compared to other molecule- and dust-forming novae inrecent years. The dust temperature and mass at two epochs have been estimatedfrom spectral energy distribution (SED) fits to infrared photometry.

V2676 Oph: Estimating physical parameters of a moderately fast nova